T Tauri candidates and accretion rates using IPHAS: method and application to IC 1396

2011/03/08 by Geert Barentsen, Jorick S. Vink, J. S. Vink +8 · 2 citations
Physics and Astronomy · #Accretion (finance) #Accretion disc #Astro and Planetary Science #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Galactic plane #Physics #Stars #Stellar, planetary, and galactic studies #T Tauri star #Telescope #astro-ph.GA #astro-ph.SR

paper · pdf · doi:10.1111/j.1365-2966.2011.18674.x

Accepted 8 March 2011 for publication in MNRAS

arxiv created 2011/03/08 · openalex publication_date 2011/05/20 · arxiv updated 2015/05/27 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

The definitive version can be found at : http://onlinelibrary.wiley.com/ Copyright Royal Astronomical Society

Citations

• WWW Database of Models of Accretion Disks Irradiated by The Central Star
• The Cradle of the Solar System
• Accretion in Young Stellar/Substellar Objects
• X‐Ray Study of Triggered Star Formation and Protostars in IC 1396N
• JHKLM photometry - Standard systems, passbands, and intrinsic colors
• Binarity as a Key Factor in Protoplanetary Disk Evolution: Spitzer Disk Census of the η Chamaeleontis Cluster
• The T Tauri Phase Down to Nearly Planetary Masses: Echelle Spectra of 82 Very Low Mass Stars and Brown Dwarfs
• SEQUENTIAL STAR FORMATION IN A COMETARY GLOBULE (BRC37) OF IC1396
• SpitzerMIPS 24 μm Detection of Photoevaporating Protoplanetary Disks
• Disk Frequencies and Lifetimes in Young Clusters
• Can Photoevaporation Trigger Planetesimal Formation?
• The Two Micron All Sky Survey (2MASS)

Cited by

• TheHerschel/PACS view of the Cep OB2 region: Global protoplanetary disk evolution and clumpy star formation
• CSI 2264: Simultaneous optical and X-ray variability in pre-main sequence stars